Table 5
Corrected magnitudes archival data of κ And b using κ And ATLAS atmospheric model.
| Date | Instrument | Band | Magnitudea | Reference |
|---|---|---|---|---|
| 2012-01/2012-07 | Subaru/HiCIAO | J | 15.850 ± 0.211 | Carson et al. (2013) |
| Subaru/HiCIAO | H | 14.923 ± 0.122 | Carson et al. (2013) | |
| Subaru/HiCIAO | Ks | 14.304 ± 0.083 | Carson et al. (2013) | |
| Subaru/IRCS | L′ | 13.12 ± 0.09b | Carson et al. (2013) | |
| 2012-10-06 | LBT/LMIRCam | M′ | 13.23 ± 0.30 | Bonnefoy et al. (2014) |
| 2012-10-30 | Keck/NIRC2 | L′ | 13.14 ± 0.09 | Bonnefoy et al. (2014) |
| 2012-11-03 | Keck/NIRC2 | Ks | 14.34 ± 0.15 | Bonnefoy et al. (2014) |
| Keck/NIRC2 | NB_4.05c | 13.00 ± 0.21 | Bonnefoy et al. (2014) | |
| 2016-11-12 | Subaru/CIAO | H | 14.63 ± 0.06d | Kühn et al. (2018) |
| 2016-07-18 | Subaru/CIAO | Y | 17.04 ± 0.15b | Uyama et al. (2020) |
Notes. (a)Apparent magnitudes in the Vega system. (b)We did not re-estimate these magnitudes since they were flux-calibrated using a different star. (c)The filter corresponds to the Brα narrow band with λc = 4.05 μm. (d)We did not include this magnitude in our study, but we included the transformed contrast to magnitude and only included the uncertainty of our ATLAS spectrum.
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